Near Horizon Geometry of Extreme Black Holes and Colliding Waves
Mustafa Halilsoy
TL;DR
This paper explores the connection between the near horizon geometries of extreme black holes and colliding gravitational waves, illustrating the correspondence with examples like Kerr and Kerr-Newman black holes.
Contribution
It extends the black hole-colliding wave correspondence to include near horizon geometries of rotating black holes with cross polarization.
Findings
Near horizon geometries of extreme Kerr and Kerr-Newman black holes are analogous to colliding wave solutions.
The correspondence applies to rotating black holes with cross polarization.
The study broadens the understanding of black hole and wave interactions in general relativity.
Abstract
The correspondence between black holes and colliding waves extends to cover the near horizon geometry of rotating black holes and colliding waves with cross polarization. Extreme Kerr and Kerr-Newman geometries are given as examples.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Pulsars and Gravitational Waves Research · Astrophysical Phenomena and Observations